NGC 1578 is a spiral galaxy in the constellation of Dorado. Its velocity with respect to the cosmic microwave background is 6,166±26 km/s, which corresponds to a Hubble distance of 296.6 ± 20.8 Mly (90.94 ± 6.39 Mpc). It was discovered by British astronomer John Herschel on 27 December 1834. NGC 1578 is an active galactic nucleus candidate, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
Supernovae Three supernovae have been observed in NGC 1578:
SN 2013fz (Type Ia, mag. 15.1) was discovered by Stuart Parker as part of the Backyard Observatory Supernova Search (BOSS) on 2 November 2013. SN 2014cd (Type Ia, mag. 15.9) was discovered by Stuart Parker as part of the Backyard Observatory Supernova Search (BOSS) on 9 August 2014. SN 2025absv (Type II-P, mag. 18.816) was discovered by ATLAS on 23 October 2025.
See also List of NGC objects (1001–2000)
References
External links Media related to NGC 1578 at Wikimedia Commons NGC 1578 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


